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SCUSHIFT
- Correct for data shift error in demodulated data files
- Description:
- This script corrects for the DAQ communications error and shifts
the data from ADC cards along by a specified amount.
Since all channels are read from a particular ADC card but only some
of them are actually stored in the demodulated data file, the shift
may result in fewer bolometers being stored for a given sub-instrument.
- Usage:
- scushift [-h] NDF card shift
- Parameters:
-
-
-h
-
Help information
-
NDF (Given)
-
The input files to be modified.
-
card
-
The letter identifying the A-to-D card (allowed values are A to I)
-
shift
-
The number of bolometers to shift by. A negative shift moves
D1 to D16 (for example) and a positive shift D1 to D2. In most
cases a negative shift is required (usually
).
- Examples:
-
- scushift test i -2
- Move the I card data of test.sdf by minus 2 bolometers
- scushift test2 h 1
- Move the H-card data by plus 1 bolometer.
- Notes:
- extinction must not have been run on the input NDF.
- Arguments are requested if they are missing from the command line
- If the system stores channels 1,2,3,6,7,8,10 but we know that we
have a shift of
in the system (ie an extra byte is present).
This implies that we have actually stored channels 16,1,2,5,6,7,9
and if only bolometers 1,2,6,7 are from the required sub-instrument
we have to throw away data from channels 15,5 and 9.
- The DAQ hardware fault always introduced extra bytes and therefore
a negative shift should be used in scushift.
- Currently photometry data is not corrected properly (the PHOT_BB
extension is not modified so the correct bolometer will not be
extracted by scuphot). This can be overcome by using the
ALLBOLS parameter in scuphot.
Next: SDIP - Reduces and displays skydip data
Up: Complete routine descriptions
Previous: SCUSETENV - Set the startup environment variables for SURF
SURF -- SCUBA User Reduction Facility
Starlink User Note 216
T. Jenness, J. F. Lightfoot
Joint Astronomy Centre, Hilo, Hawaii
3 April 2003
E-mail:ussc@star.rl.ac.uk
Copyright © 1997-2000,2003 Particle Physics and Astronomy Research Council